Nonthermal radiative transfer of oxygen 98.9 nm ultraviolet emission: Solving an old mystery-Reference-Cited by-同舟云学术

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Nonthermal radiative transfer of oxygen 98.9 nm ultraviolet emission: Solving an old mystery

Published:2015-12 Issue:12 Volume:120 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Hubert B.¹,Gérard J.‐C.¹,Shematovich V. I.²,Bisikalo D. V.²,Chakrabarti S.³,Gladstone G. R.⁴

Affiliation:

1. Laboratory for Planetary and Atmospheric Physics University of Liege Liege Belgium

2. Institute of Astronomy Russian Academy of Sciences Moscow Russia

3. Lowell Center for Space Science and Technology University of Massachusetts Lowell Massachusetts USA

4. Southwest Research Institute San Antonio Texas USA

Funder

Office of Naval Research

National Science Foundation

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2014JA020835

Reference68 articles.

1. The OI 989-Å tropical nightglow

2. A reexamination of important N2cross sections by electron impact with application to the dayglow: The Lyman-Birge-Hopfield Band System and N I (119.99 nm)

3. A model of nitric oxide in the lower thermosphere

4. Dielectronic recombination to normal nitrogen and oxygen ions

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Quantifying the Electron Energy of Mars Aurorae Through the Oxygen Emission Brightness Ratio at 130.4 and 135.6 nm;Journal of Geophysical Research: Planets;2024-03

2. A Comparative Analysis of the OI 130.4‐nm Emission Observed by NASA's TIMED Mission Using a Monte Carlo Radiative Transfer Model;Journal of Geophysical Research: Space Physics;2020-01

3. Characteristics of Mars UV Dayglow Emissions From Atomic Oxygen at 130.4 and 135.6 nm: MAVEN/IUVS Limb Observations and Modeling;Journal of Geophysical Research: Space Physics;2019-06

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